SDSS J001153.08-064739.1: most likely SU UMa star
Josch Hambsch has recored a 0.2 mag hump.
Although the baseline is one orbital cycle, the profile
and amplitude suggest a superhump. This object is
very interesting since it is in the period gap
and has an evolved secondary. The reported mass ratio
is above 0.25 and the detection of superhumps is
great astrophysical importance. Continued observations
are encouraged.